The Jovian D/H problem can be approached three ways: a) D &
H Ly-\alpha, Ly-\beta, b) CH3D and CH4, and c) HD
and H2 (from ISO/Galileo probe). The same atmospheric
model should provide the same D/H ratio regardless of
technique used. We have extensively studied the D/H problem
utilising these approaches and report the results of our
analysis which compare very favourably with various
observations in most cases.

The author(s) of this abstract have provided an email address
for comments about the abstract:
chris@nimbus.yorku.ca